Erosional processes, ages and stratigraphic sequence in the Hydraotes Chaos Region, Mars: Observations of the HRSC Camera aboard Mars Express R. Wagner2, 1 B. Schreiner , 1Institute of Geosciences, Freie Universitaet, Berlin, Germany 1 S. van Gasselt , 2Institute of Planetary Research, DLR Berlin, Germany G. Neukum1, and the HRSC Co-I Team Acknowledgements: U. Wolf2 for crater counting Regional setting: topography and geology Regional setting: topography and geology HRSC coverage (up to orbit 1394) Regional setting: topography and geology Procedure ♦ Identify and map geologic / morphologic units ♦ Determine heights of morphologic units ♦ Crater counts on geologic / morphologic units: --> derive stratigraphic sequence ♦ Application of the cratering chronology model by Hartmann and Neukum (2001) --> absolute time scales; duration of processes Geologic units Hydraotes Chaos: Mesas / Medium level Xanthe Terra: plains Top level Geologic units Hydraotes Chaos: Hydraotes Chaos: Mesas & valley floor / Bright floor Lowest level Geologic units Hydraotes Chaos: Dark floor Determination of heights Hydraotes Chaos: Perspective view Determination of heights Heights of distinct mesas: Parallax measurements between HRSC nadir and stereo channel ÆAllows to find height values for small features below the spatial resolution Absolute calibration of parallaxes with MOLA DTM Height range: -5100 m (floor) to 2500 m (red color) Cratering chronology Stratigraphy and ages Xanthe Terra / Hydraotes Chaos: Top level Xanthe Terra: ~3.9 Gyr Erosional episode #1: ~1.6 Gyr Stratigraphy and ages Xanthe Terra / Hydraotes Chaos: Medium level Xanthe Terra: ~3.9 Gyr Erosional episode #1: ~1.6 Gyr Stratigraphy and ages Xanthe Terra / Hydraotes Chaos: Medium level Erosional episode #2: ~0.5 Gyr Stratigraphy and ages Xanthe Terra / Hydraotes Chaos: Lowest level Erosional episode #2: ~0.5 Gyr Stratigraphy and ages Xanthe Terra / Hydraotes Chaos: Lowest level Erosional episode #3: ~0.4 Gyr to ~0.2 Gyr Conclusions ♦ Wide range of high- and lowland morphologies (bright & dark floors, small buttes, angular mesas) ♦ Morphological features resemble terrestrial landforms dissected and eroded by water ♦ Elevation levels from -5100 m (floors) to 2500 m ♦ So far unclear whether different elevation levels due to: (1) Surface removal & subsequent abrasion (2) Removal of subsurface material & block tilting Conclusions ♦ Xanthe Terra: plains-forming volcanism, 3.9 Gyr ♦ Top level mesas: long-lasting erosional process, ceased or slowed down about 1.6 Gyr ago ♦ Medium level mesas: erosional process, ceased (or slowed down) about 500 Myr ago ♦ Low level mesas, floors: erosional process, ceased 400 - 200 Myr ago Conclusions Medium Low Top Outflow channels Simud & Tiu Xanthe Terra Vallis Hydraotes Chaos mesas.